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Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Development of liquid xenon scintillation detector for new experiment to search for   e 

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Presentation on theme: "Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Development of liquid xenon scintillation detector for new experiment to search for   e "— Presentation transcript:

1 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Development of liquid xenon scintillation detector for new experiment to search for   e  decays Development of liquid xenon scintillation detector for new experiment to search for   e  decays W.Ootani a, T.Doke c, T.Haruyama d, T.Ishida a, A.Maki d, T.Mashimo a, S.Mihara a, T.Mitsuhashi a, T.Mori a, H.Nishiguchi a, S.Orito b, K.Ozone a, R.Sawada c, S.Suzuki c, K.Terasawa c, M.Yamashita c, J.Yashima d, and T.Yoshimura c a International Center for Elementary Particle Physics, University of Tokyo, Tokyo, Japan b Department of Physics, School of Science, University of Tokyo, Tokyo, Japan c Advanced Research Inst. for Science and Engineering, Waseda University, Tokyo, Japan 4 High Energy Accelerator Research Organization (KEK), Tsukuba, Japan

2 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Physics motivations Event signature Back to back Time coincident E e = E  = 52.8MeV Lepton-family-number nonconserving process Forbidden in the standard model Sensitive to physics beyond the standard model SUSY-GUT, SUSY+ν R, … Present experimental bound BR(  +  e +  ) < 1.2 x 10 - 11 (MEGA experiment, 1999) New experiment with a sensitivity of BR~10 -14 planned at PSI Event signature Back to back Time coincident E e = E  = 52.8MeV Lepton-family-number nonconserving process Forbidden in the standard model Sensitive to physics beyond the standard model SUSY-GUT, SUSY+ν R, … Present experimental bound BR(  +  e +  ) < 1.2 x 10 - 11 (MEGA experiment, 1999) New experiment with a sensitivity of BR~10 -14 planned at PSI   e  decay μ+μ+ e+e+ γ

3 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Physics motivations, cont’d SU(5) SUSY-GUT predicts BR (   e  ) = 10 -15 - 10 - 13 (SO(10) SUSY-GUT: even larger value 10 -13 - 10 -11 ) SU(5) SUSY-GUT predicts BR (   e  ) = 10 -15 - 10 - 13 (SO(10) SUSY-GUT: even larger value 10 -13 - 10 -11 ) J. Hisano et al., Phys. Lett. B391 (1997) 341 Our goal

4 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 New   e  experiment at PSI Sensitivity down to BR~10 -14 World’s most intense DC muon beam at PSI Liquid xenon gamma detector Positron spectrometer with gradient magnetic field Thin superconducting magnet Engineering/physics run will start in 2003 Sensitivity down to BR~10 -14 World’s most intense DC muon beam at PSI Liquid xenon gamma detector Positron spectrometer with gradient magnetic field Thin superconducting magnet Engineering/physics run will start in 2003

5 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 LXe gamma-ray detector Detector design Active volume of LXe: 800 liter Scintillation light is collected by ~800 PMTs immersed in LXe Effective coverage: ~ 35% Detector design Active volume of LXe: 800 liter Scintillation light is collected by ~800 PMTs immersed in LXe Effective coverage: ~ 35% Detector requirements: Excellent energy-, timing-, and position resolutions Detector requirements: Excellent energy-, timing-, and position resolutions Liquid xenon scintillation detector 

6 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Liquid xenon scintillator Mass number131.29 Density3.0 g/cm 3 Boiling and melting points 165 K, 161 K Energy per scintillation photon 21.7 eV for  18.1 eV for  Radiation length2.77 cm Decay time4.2 nsec (fast) 22 nsec (slow) 45 nsec (recombi.) Scintillation light wave length 175 nm Refractive index1.57 LXe properties High light yield (75% of NaI(Tl)) Fast signals  avoid accidental pileups Spatially uniform response  no need for segmentation High light yield (75% of NaI(Tl)) Fast signals  avoid accidental pileups Spatially uniform response  no need for segmentation

7 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Photomultiplier Dynode structureMetal channel Photo cathodeRb-Cs-Sb WindowQuartz Quantum efficiency~10 % PMT size 57 mm  Effective area 46 mm  PMT Length32 mm Typical H.V.1000 V Current amplification10 6 - 10 7 TTS0.3 ns typ. Dynode structure Hamamatsu R6041Q Successfully operated in liquid xenon

8 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 First prototype of LXe detector 32 x PMTs Active LXe volume 116 x 116 x 174 mm 3 (2.3liter) Energy-, Position-, and Timing resolutions for gamma up to 2MeV 32 x PMTs Active LXe volume 116 x 116 x 174 mm 3 (2.3liter) Energy-, Position-, and Timing resolutions for gamma up to 2MeV

9 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Results from first prototype Energy Simple extrapolations from the results and simulation studies imply,  energy ~ 1%,  position ~ a few mm,   time ~ 50psec  for 52.8MeV gamma from   e  Simple extrapolations from the results and simulation studies imply,  energy ~ 1%,  position ~ a few mm,   time ~ 50psec  for 52.8MeV gamma from   e  Should be verified with larger detector for higher energy(~50MeV) gamma rays Should be verified with larger detector for higher energy(~50MeV) gamma rays

10 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Second prototype Second prototype successfully constructed

11 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Second prototype, cont’d Purposes of second prototype Demonstrate performance of planned full-scale detector by using high energy  (Energy-, position-, time- resolutions) Check of cryogenics and other detector components Measurement of absorption length of scintillation light in LXe Purposes of second prototype Demonstrate performance of planned full-scale detector by using high energy  (Energy-, position-, time- resolutions) Check of cryogenics and other detector components Measurement of absorption length of scintillation light in LXe Second prototype (large prototype) Part of full-scale detector World’s largest LXe scintillation detector! A total of 120 liter liquid xenon (active volume of 69 liter) Viewed by 228 PMTs Large enough to test with ~50MeV  LEDs and  sources ( 241 Am) implemented for calibration Second prototype (large prototype) Part of full-scale detector World’s largest LXe scintillation detector! A total of 120 liter liquid xenon (active volume of 69 liter) Viewed by 228 PMTs Large enough to test with ~50MeV  LEDs and  sources ( 241 Am) implemented for calibration

12 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Cryogenic system Pulse-tube refrigerator Cooling power of pulse-tube refrigerator Xenon is liquefied by heat exchange with LN 2. Liquid is kept stably with pulse-tube refrigerator after liquefaction. Measured cooling power at 165K ~ 70W ( total heat load of the prototype detector ~ 52W) No serious problem during over 50days detector operation! Xenon is liquefied by heat exchange with LN 2. Liquid is kept stably with pulse-tube refrigerator after liquefaction. Measured cooling power at 165K ~ 70W ( total heat load of the prototype detector ~ 52W) No serious problem during over 50days detector operation! Cold head

13 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Purification system Impurity in LXe such as H 2 O, O 2 is critical.  absorption of scintillation light Two Purification filters employed Oxisorb filter (Messer Griesheim) Zr-V-Fe getter (SAES geeters, MonoTorr) Flushing chamber by hot xenon gas circulation prior to liquefaction Xenon vapor gas circulated during detector operation Monitoring impurity concentration using mass spectrometer Impurity in LXe such as H 2 O, O 2 is critical.  absorption of scintillation light Two Purification filters employed Oxisorb filter (Messer Griesheim) Zr-V-Fe getter (SAES geeters, MonoTorr) Flushing chamber by hot xenon gas circulation prior to liquefaction Xenon vapor gas circulated during detector operation Monitoring impurity concentration using mass spectrometer

14 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 PMT calibration PMT calibration by using LEDs. Gain estimation with ~3% accuracy. PMT calibration by using LEDs. Gain estimation with ~3% accuracy. LED Gain curve Accuracy in gain estimation

15 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Gamma beam test Performance test of large prototype using high-energy gamma rays Laser Compton backscattering facility at TERAS electron storage ring of AIST, Tsukuba, Japan Gamma-ray beam with energy up to 40MeV Energy resolution evaluated by spread of Compton edge Position reconstructed by PMT output distribution with proper collimator Timing reconstructed by averaging arrival time Performance test of large prototype using high-energy gamma rays Laser Compton backscattering facility at TERAS electron storage ring of AIST, Tsukuba, Japan Gamma-ray beam with energy up to 40MeV Energy resolution evaluated by spread of Compton edge Position reconstructed by PMT output distribution with proper collimator Timing reconstructed by averaging arrival time

16 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Gamma beam test, cont’d Energy spectrum of gamma beam with 1mm  collimator (simulation)

17 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Gamma beam test, cont’d Studies with high-energy gamma beam started Various detector components worked well (refrigerator, feedthrough, PMT holder, etc.) 40MeV gamma successfully observed Data analysis to evaluate detector resolutions(energy, spatial, timing) in progress Essential parameters such as QE of PMTs, absorption length of scintillation light in LXe, etc are needed  separate experiments to measure such parameters going on Studies with high-energy gamma beam started Various detector components worked well (refrigerator, feedthrough, PMT holder, etc.) 40MeV gamma successfully observed Data analysis to evaluate detector resolutions(energy, spatial, timing) in progress Essential parameters such as QE of PMTs, absorption length of scintillation light in LXe, etc are needed  separate experiments to measure such parameters going on ~40MeV gamma event

18 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Design work on full-scale detector Full-scale detector Active volume of 800 liter Viewed by ~800 PMTs Full-scale detector Active volume of 800 liter Viewed by ~800 PMTs Vessel design Vessel design almost finalized (Heat load calculation, mechanical analysis) PMT frame design Refrigerator design Vessel design almost finalized (Heat load calculation, mechanical analysis) PMT frame design Refrigerator design

19 Wataru Ootani, ICEPP, Univ. of Tokyo SORMA X, May 21, 2002 Summary New experiment to search for   e  with a sensitivity of BR~10 -14 planned at PSI. Novel liquid xenon scintillation detector for the experiment under development. Large prototype with an active volume of 69 liter constructed. The prototype operated successfully over 50days. Studies with gamma beam up to 40MeV at laser Compton backscattering facility started. 40MeV gamma event successfully observed. Data analysis in progress to reliably evaluate energy-, position-, and timing- resolutions. Separate experiments to measure essential parameters such as QE of PMTs, absorption length, etc. are going on. Design work on full-scale detector going on. New experiment to search for   e  with a sensitivity of BR~10 -14 planned at PSI. Novel liquid xenon scintillation detector for the experiment under development. Large prototype with an active volume of 69 liter constructed. The prototype operated successfully over 50days. Studies with gamma beam up to 40MeV at laser Compton backscattering facility started. 40MeV gamma event successfully observed. Data analysis in progress to reliably evaluate energy-, position-, and timing- resolutions. Separate experiments to measure essential parameters such as QE of PMTs, absorption length, etc. are going on. Design work on full-scale detector going on. For more info, see http://meg.icepp.s.u-tokyo.ac.jp For more info, see http://meg.icepp.s.u-tokyo.ac.jp/


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